Titlebook: Energy Transfer and Dissipation in Plasma Turbulence; From Compressible MH Yan Yang Book 2019 The Editor(s) (if applicable) and The Author(

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Claudia Lucia Velandia Gomez,Michele Girottoery detail of plasmas from the largest to the smallest spatial and temporal scales. The amount of information contained in the many-body distribution function is vast, and as a consequence it is very hard to directly deal with the Liouville equation.

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Torsten Tomczak,Sven Reinecke,Alfred Kussr than the MHD fluid scales, i.e., at kinetic scales, means that characterizing the properties with MHD approximation does not work, but rather more refined models embodying kinetic plasma effects are required.

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Theoretical Modelling,ery detail of plasmas from the largest to the smallest spatial and temporal scales. The amount of information contained in the many-body distribution function is vast, and as a consequence it is very hard to directly deal with the Liouville equation.

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,Energy Transfer and Dissipation in?Collisionless Plasma Turbulence,r than the MHD fluid scales, i.e., at kinetic scales, means that characterizing the properties with MHD approximation does not work, but rather more refined models embodying kinetic plasma effects are required.

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Introduction,Plasma turbulence is ubiquitous in space and astrophysical flows. For example, the solar wind emitting from the sun into interplanetary space, one of the most studied natural plasmas, is in a turbulent state.